MMS data from a 2023 CME show elevated electron temperatures with superthermal tails, depleted mid-energy electrons, and weak MHD-like turbulence with reduced intermittency in the rare sub-Alfvénic solar wind at 1 AU.
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The paper reviews electron transport in tangled magnetic fields, including creation via turbulence, modulation by instabilities, trapping, cross-field diffusion, and energization.
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MMS Insights into CME Driven Sub-Alfv\'enic Solar Wind at 1 AU
MMS data from a 2023 CME show elevated electron temperatures with superthermal tails, depleted mid-energy electrons, and weak MHD-like turbulence with reduced intermittency in the rare sub-Alfvénic solar wind at 1 AU.
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Transport of electrons in tangled magnetic fields
The paper reviews electron transport in tangled magnetic fields, including creation via turbulence, modulation by instabilities, trapping, cross-field diffusion, and energization.